The galaxy presents as a fairly smooth, elliptical-like structure, exhibiting a high degree of central concentration. The light profile appears to be dominated by an older stellar population, indicated by the yellowish-orange hue, which likely corresponds to evolved red giant stars. There is a subtle color gradient, with the central region appearing slightly more yellow and the outer regions exhibiting a marginally redder tone. There is little evidence of spiral arms or prominent dust lanes; instead, there is a gradual decrease in luminosity from the bright core outwards. No obvious signs of ongoing major star formation are apparent in the visible bands, indicating a relatively quiescent galaxy in terms of current star formation activity. Based on the data, there is a chance that this galaxy is experiencing minor disturbances. The galaxy appears to be roughly round in shape, but not perfectly spherical.