This galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright core that gradually diffuses outward. There's a slight elongation, leaning towards a round shape, but not perfectly spherical.

The color profile shows a mix of wavelengths, with the central region appearing slightly redder than the outer edges, which have a bluer hue. There are no clearly defined spiral arms or prominent dust lanes visible, suggesting either a lack of active star formation in well-defined spiral arms, or potentially obscuration due to the viewing angle. 

There is a faint suggestion of some minor disturbance in the overall symmetry. Further investigation with higher resolution imaging could help determine if this is an interaction with a smaller galaxy, or an internal feature.
