The galaxy presents as an elongated, diffuse structure with a relatively smooth overall appearance. Its central region exhibits a higher surface brightness, gradually fading towards the edges, suggesting a centrally concentrated stellar population. There is a faint, extended halo surrounding the brighter core, implying a considerable spatial extent. The galaxy appears to lack a well-defined spiral arm structure or prominent dust lanes. There is also evidence of a possible minor disturbance or interaction, as one edge appears to be slightly disrupted. Color gradients are observed, with the central regions appearing slightly more yellow or red compared to the bluer hues in the outer regions, indicative of differing stellar populations or dust obscuration. Overall, the galaxy likely falls within the category of lenticular or possibly an elliptical galaxy with some signs of past or ongoing interaction.
