The galaxy appears to be relatively smooth in texture and elliptical in shape. The central region exhibits a high degree of concentration, with luminosity decreasing outwards. A slight elongation is visible along its major axis, departing marginally from a perfectly circular profile. There may be a minor disturbance within the structure of the galaxy. A secondary object is nearby and slightly offset, possibly a smaller galaxy or a tidal feature resulting from a gravitational interaction. The color profile displays a yellow/red hue in the center, suggesting older stellar populations, with bluer components in areas further from the core, indicating star formation. The overall morphology suggests the object has undergone or is currently undergoing a merger event, potentially disrupting the smooth distribution of matter typically observed in elliptical galaxies.
