The galaxy presents as a moderately bright, elliptical-like structure with a noticeable central bulge. Its overall form suggests a somewhat spheroidal shape, though slightly elongated, with a smooth, diffuse light distribution throughout. There is no distinct spiral arm structure visible. The core region appears to be the brightest and most concentrated area of the galaxy. The galaxy's color profile leans toward redder hues, indicative of an older stellar population. The lack of significant blue regions suggests relatively low ongoing star formation activity. There is some minor indication of a possible tidal disturbance or interaction.
