The galaxy presents as a relatively luminous object with a discernible reddish-yellow hue. It is of intermediate size relative to other background objects within the field. The morphology appears disturbed, possibly indicating ongoing or recent merger activity. There is a primary, somewhat rounded central component that is smooth in appearance, with a fainter, elongated secondary component. The shape departs slightly from a perfect sphere, exhibiting a mild ellipticity. Light distribution shows no distinct spiral arm structure. Based on the apparent color profile, stellar populations are most likely dominated by older stars with ongoing, but relatively low star formation.
