The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. The central region exhibits a bright, concentrated bulge, suggesting a high density of stars. Proceeding outward from the core, the light gradually diffuses with a smooth profile, and the outer regions begin to diminish into the background. There seems to be a slight asymmetry in the outer regions. A subtle color gradient is present, with the core trending towards yellow/white and the surrounding disk displaying slight redder hues, indicating older stellar populations towards the outer regions. It appears to be isolated, without any obvious signs of recent or ongoing major mergers.