The galaxy presents as a slightly elongated structure, generally smooth in appearance but with hints of internal features. The color distribution suggests a dominant older stellar population, concentrated toward the central region, which exhibits a yellowish hue. There is a subtle color gradient, becoming slightly bluer towards the outer regions of the galaxy which indicates some recent star forming activity. The galaxy appears to be well defined but not perfectly circular, trending towards a cigar shape. There are no obvious signs of major disturbances or ongoing mergers and interactions with other galaxies. There is no clear spiral arm structure or a strong central bar visible. Overall, the galaxy exhibits characteristics of a relatively evolved system with evidence of a fairly high stellar mass and relatively low star formation activity.
