This galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution. The central region is noticeably brighter, suggesting a concentration of stars and potentially a supermassive black hole. The galaxy's overall shape is somewhat elongated, deviating slightly from a perfect sphere. There is little evidence of spiral arms or distinct disk structures. The color profile indicates a dominance of older stellar populations, with a general yellowish hue. No significant signs of ongoing major mergers or tidal disturbances are readily apparent, although subtle asymmetries may indicate minor past interactions. The faint outer regions suggest a gradual decline in stellar density with increasing radius. Overall, this galaxy presents a morphology consistent with a well-evolved system undergoing relatively little active star formation.
