The galaxy presents a generally smooth morphology, with a somewhat elliptical shape. The light distribution appears concentrated toward the center, with a gradual falloff in brightness towards the edges. There is minimal indication of spiral arms or distinct features typically associated with actively star-forming regions. The galaxy exhibits a subtle color gradient, appearing bluer towards the core and slightly redder in the outer regions. This suggests that the central regions may have a higher concentration of younger, hotter stars, or potentially a more active galactic nucleus, although the resolution is insufficient to confirm the latter. The overall appearance points towards a relatively evolved system, likely an elliptical or lenticular galaxy, with a low current rate of star formation. There is a slight asymmetry in the outer regions. Possible minor interactions with other celestial bodies may be present, but are not significant. No substantial dust lanes or major disturbances are visible.
