The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse halo or disk component, displaying a bluer color gradient compared to the bulge. This suggests the presence of a younger stellar population and possibly some ongoing star formation in the outer regions.

The overall shape appears more rounded than elongated, though there's a slight deviation from perfect circularity. There is no prominent evidence of spiral arm structures or a well-defined disk. The galaxy appears largely undisturbed, showing no obvious signs of major mergers or significant tidal interactions. Faint, subtle irregularities or minor disturbances may be present in the outer regions.
