The galaxy presents as a moderately elliptical structure, with a smooth and diffuse light distribution. It appears to be dominated by an older stellar population, inferred from its yellowish-golden hue. There is a slightly more pronounced central bulge. No distinct spiral arm features or significant dust lanes are visible, although there is some subtle colour variation across the galaxy, with perhaps slight bluer tones in the outer regions. Overall, the galaxy's morphology suggests a relatively evolved system, potentially of significant mass. There does not appear to be any signs of any merger events in the recent past.
