The galaxy presents a generally smooth morphology. It exhibits a somewhat elongated, elliptical shape, appearing as a flattened spheroid. The light distribution suggests a concentrated central bulge, with a gradual decrease in luminosity towards the outer regions. The galaxy appears to be a yellowish color, suggesting an older stellar population. There appears to be no distinct spiral arm structure or prominent dust lanes visible. The galaxy has a reddish hue, possibly indicating a relatively quiescent star formation rate. No major disturbances or signs of ongoing mergers are immediately apparent.
