The galaxy presents a roughly elliptical morphology, exhibiting a smooth light distribution with a highly concentrated central bulge. The galaxy's color profile indicates a generally redder hue, particularly towards the core, suggesting an older stellar population. There is a subtle, diffuse disk structure surrounding the central bulge, though no distinct spiral arm features are discernible. The galaxy does not appear to be undergoing any major merging events or exhibiting significant tidal disturbances. The light profile appears fairly uniform and consistent across the object, implying a relatively quiescent evolutionary state.
