The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The core is bright and yellowish-white in color, suggestive of an older stellar population. It exhibits a mostly round shape. There is an observed irregularity in its shape. There appears to be a potential minor disturbance or perhaps early stage merger occurring. There is what appears to be a bulge or core that has some overlap or physical contact with the core. This overlap of light suggests a potential interaction. Overall, this galaxy seems to have a well-defined, older population. There is potential for it to be undergoing some type of interaction, however further observation would need to take place to confirm.
