The galaxy presents as a luminous, elliptical form with a smooth, concentrated light profile. The core region exhibits a bright, yellowish hue, suggesting an older stellar population dominated by redder giants and supergiants. There appears to be a subtle color gradient extending outwards from the core, transitioning to slightly bluer tones in the outer regions of the galaxy, which could indicate the presence of younger, hotter stars at lower densities. Overall, the galaxy appears to be relatively undisturbed, lacking prominent spiral arms or significant dust lanes. The morphology suggests that this galaxy is an elliptical or lenticular type, with no indications of ongoing major merging events.