The galaxy appears elliptical in shape, exhibiting a relatively smooth and concentrated light distribution. There is a bright central bulge, suggestive of an older stellar population, with light intensity decreasing gradually outwards. Fainter, diffuse light extends beyond the bright central region. There are hints of bluer light in the outskirts, possibly indicating some level of ongoing star formation, although this is minimal. There are no signs of any significant disturbances, tidal tails, or merging activity visible in the image. Overall the galaxy presents a consistent and unperturbed structure. The estimated size of the galaxy suggests that it is a moderate sized galaxy.
