The galaxy presents a generally smooth morphology, appearing as a single, concentrated object. It exhibits a somewhat elliptical shape, leaning towards a rounded appearance but showing a slight elongation. The color profile suggests an older stellar population, with a predominantly yellowish-red hue dominating the central regions. There is a hint of bluer light at one end, perhaps indicating localized star formation in that region. While the overall structure is smooth, there are indications of possible disturbances. There is no definitive evidence of a major merger event, though the possibility of a minor interaction cannot be entirely ruled out.
