The galaxy appears to be a relatively small, elongated elliptical galaxy, classified as a cigar-shaped galaxy based on its high aspect ratio. It exhibits a smooth, featureless morphology with no obvious spiral arms or prominent disk structures. The central bulge dominates the galaxy's overall light profile, gradually fading towards the edges. There are no distinct signs of tidal disturbances or ongoing mergers, suggesting it is a relatively isolated system that is stable. There is no evidence of recent or intense star formation activity. The galaxy appears to be a mature system consisting mainly of older stellar populations.
