The galaxy presents as a moderately luminous, relatively compact system. Its overall morphology appears largely smooth with a slight elongation. The light distribution is concentrated towards the center, suggesting a high degree of central mass concentration. The color profile transitions from a yellowish central region to a redder outer halo. This color gradient implies that the stellar population in the core is dominated by older, redder stars, while the outskirts may contain a younger, bluer population or be more affected by dust reddening. There are no obvious signs of spiral arms or prominent dust lanes. Furthermore, there appears to be some level of disturbance in the surrounding area with a slight hint of some possible ongoing interactions or tidal features. The object lacks intense star-forming regions.
