The galaxy presents as a generally smooth, elliptical morphology, exhibiting a bright, concentrated core indicative of a possible central supermassive black hole. The light distribution fades gradually from the core, suggesting a well-mixed stellar population. The galaxy shows intermediate roundness in its overall shape, without a pronounced disk component. The color profile reveals a concentration of slightly bluer light in the central region, likely caused by recent star formation. The outer regions appear redder, suggesting an older stellar population. There may be a small disturbance or tidal feature in the outskirts, hinting at a possible minor interaction with a smaller galaxy in the past, but further investigation would be needed to confirm.
