The galaxy presents as a centrally concentrated, somewhat smooth structure with a generally elliptical morphology. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Diffuse, less concentrated regions surrounding the core display a more reddish tint, possibly indicating the presence of dust or a population of cooler stars. There is little evidence of distinct spiral arm structure or significant star formation activity from this view. The overall appearance is indicative of a relatively evolved system, potentially an elliptical or lenticular galaxy, with a substantial stellar mass. Subtle disturbances are not easily discernible within the galactic structure, implying a state of relative gravitational stability.
