The galaxy presents a relatively smooth morphology, with an overall elliptical appearance. It exhibits a centrally concentrated bulge, gradually fading into an extended halo. There is evidence of a faint, disky component extending from the bulge. The galaxy appears to have a slight amount of diskiness and not be perfectly smooth. The color gradients suggest the presence of an older stellar population dominating the bulge, and a younger stellar population forming in the disk. The presence of minor disturbances suggests possible interactions or recent mergers, though no prominent tidal features are visible. Overall, the galaxy appears to be a moderately massive system with ongoing, though relatively low, star formation activity. The elongated morphology may indicate an intermediate stage of morphological transformation.
