The galaxy presents a generally smooth and rounded morphology, indicative of an elliptical or S0 type galaxy. There's a noticeable concentration of light towards the center, suggesting a prominent galactic bulge. The color profile appears relatively uniform across the galaxy, with a yellowish hue. There is no evidence of spiral arms or significant dust lanes in the visible spectrum. The galaxy appears relatively isolated. The size is difficult to determine with precision, but the light distribution implies a fairly compact object. There are no signs of a major ongoing merger. There may be a very slight asymmetry, but this could also be a product of image processing and the resolution provided. There is no blue light, meaning that the galaxy is mostly composed of older stars with a low star formation rate.