The galaxy appears as a centrally concentrated object with a generally smooth light distribution. The core region exhibits a yellowish hue, suggesting an older stellar population. The galaxy fades smoothly toward its outer edges, showing a gradual decrease in surface brightness. There is a slight elongation in its shape but no easily discernible disk or spiral arm structures. There does not appear to be any sign of ongoing major merging activity or significant tidal disturbances in the immediate vicinity of the galaxy.
