The galaxy appears as a centrally concentrated object with a smooth, diffuse profile. The light distribution suggests a relatively spheroidal morphology, with no obvious spiral arm structures or prominent dust lanes visible. The galaxy exhibits a color gradient, appearing brighter and slightly redder towards the core, transitioning to a fainter and bluer hue in the outer regions. There is no discernible evidence of any major ongoing mergers or significant tidal disturbances affecting its structure. The overall appearance suggests a mature system, likely an elliptical or lenticular galaxy, with a relatively low star formation rate. The light is generally smooth and even, indicating a lack of significant recent starburst activity or prominent HII regions.
