The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile appears to gradually decrease in intensity from the core outwards, without any distinct spiral arms or bar structures immediately visible. The overall shape is neither perfectly spherical nor highly elongated, suggesting an intermediate elliptical classification.

The color distribution is not uniform across the galaxy. The central region exhibits a yellowish-white hue, indicative of an older stellar population. This color transitions to a slightly bluer tint in the outer regions, possibly suggesting the presence of younger, hotter stars or ongoing star formation at lower levels. 

There are no obvious signs of significant tidal disturbances or interactions with other galaxies, though it's possible that minor past interactions could have contributed to the current morphology. There do not appear to be strong features indicative of a recent or ongoing merger event.
