The galaxy presents a somewhat elliptical morphology. The light distribution appears relatively smooth, with a central bulge that is significantly brighter and more concentrated than the surrounding regions. The color profile suggests a redder core, transitioning to slightly bluer hues in the outer disk or halo. There is no clear evidence of spiral arm structure or significant dust lanes from this perspective. The object's overall appearance is suggestive of a galaxy that is dominated by an older stellar population, particularly in its central regions. No signs of active merging or tidal disturbances are obviously visible.
