The galaxy presents as an elliptical morphology with moderate features. There appears to be a concentrated central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population dominating that region. The overall shape is oblong with a slight elongation. Peripheral regions display a bluer tint, possibly suggesting the presence of younger, hotter stars. The galaxy shows some indications of disturbed morphology, possibly indicative of a minor gravitational interaction.  No clear spiral arm structure is apparent. Overall, the galaxy exhibits a moderate degree of smoothness, with a notable absence of strong star-forming regions based on the relative lack of intense blue or pink coloration.
