The galaxy exhibits a generally smooth morphology, with no discernible spiral arm structures or prominent dust lanes visible. The light distribution appears centrally concentrated with a gradual decrease in luminosity outwards from the core. Its shape is nearly circular, presenting a fairly round appearance on the sky. There is no visually obvious evidence of any major ongoing merger activity or significant tidal disturbances that may indicate recent interaction with another galaxy. The galaxy's color is primarily a yellowish-orange hue. This suggests a dominant stellar population of older, redder stars, potentially indicating a relatively low star formation rate within the galaxy.