The galaxy presents a somewhat elliptical morphology, exhibiting a relatively smooth light distribution with a hint of asymmetry. A bright, concentrated central bulge is apparent, fading outwards into a less defined disk. There may be a weak tidal feature to the north of the bulge, suggesting past or ongoing gravitational interaction. The color profile indicates a concentration of older stars, primarily in the central regions, while the outer regions display slightly bluer hues, suggesting a more diverse stellar population and potential for moderate star formation. The galaxy's structure is suggestive of a transition between elliptical and spiral types.
