The galaxy exhibits a generally smooth morphology, with a dominant central bulge region. There is faint indication of a disk structure, though any spiral arms are not clearly defined in this observation. The overall shape appears somewhat elliptical, transitioning towards a more lenticular form. There is no significant evidence of tidal tails, merging events, or major disturbances.

The galaxy's light distribution is concentrated towards the core, with a gradual fall-off in intensity towards the outer regions. Color gradients are subtle, with the central regions appearing bluer compared to the slightly redder outer regions. The overall color suggests it is populated by both young and old stars, with the presence of some ongoing star formation. The lack of major dust lanes or prominent star-forming regions indicates the star formation rate is relatively low.

The galaxy displays no sharp edges or distinct features, suggesting a lack of recent, violent interactions. This implies that the system is relatively settled and has undergone significant morphological evolution.
