This galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a higher density of stellar populations and potentially a supermassive black hole. The light distribution gradually fades outward from the core.

The galaxy's overall color profile indicates a predominantly older stellar population, exhibiting a slight redder hue in the outer regions compared to the more blueish-white central area. There is subtle evidence of minor disturbances or asymmetries in the outer envelope, which may be indicative of past minor merger events or tidal interactions. The galaxy displays an intermediate ellipticity, neither perfectly spherical nor highly elongated, but clearly not a spiral. I am not able to detect clearly defined spiral arms or a well-defined disk structure within the limits of resolution afforded by the image. The image shows no clear signs of ongoing major mergers, but some potential minor disturbances are present.
