The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a concentrated luminosity, characterized by a yellowish-orange hue. This suggests a relatively older stellar population dominating the core, with limited ongoing star formation. Moving outwards from the center, the color gradient shifts towards a paler white and somewhat bluish tone, although these outer regions remain diffuse. The galaxy lacks any significant visible spiral arm structure or prominent dust lanes. There are hints of potential minor disturbances or tidal features, but these are not distinct. Overall, the galaxy appears to be a relatively massive, early-type system, potentially undergoing quiescent evolution with a low rate of star formation.
