The galaxy presents a mostly smooth morphology with a concentration of light toward the center, indicating a prominent bulge. While the overall structure is generally smooth, subtle irregularities suggest potential gravitational interactions or internal dynamics. The shape is somewhat elliptical and not perfectly circular, leaning towards an 'in between' classification.

Faint, extended features are visible, possibly indicative of tidal tails or debris resulting from minor disturbances. The color profile suggests a population of older stars dominating the galaxy, supported by a reddish hue with traces of bluer star formation regions. There is evidence of a potential interaction or merger with another galaxy or smaller object, with a portion of the light appearing separate from the main body of the galaxy. Overall, the galaxy appears to be in a late stage of evolution, moving toward becoming a spheroid or elliptical system, with only minor ongoing activity.
