The galaxy presents as a somewhat diffuse object, with a moderately flattened elliptical morphology. There appears to be a central concentration of light, though it lacks a distinct, well-defined nucleus. The galaxy exhibits a color gradient, appearing bluer in the outer regions and trending toward a more reddish-yellow hue in the central regions. Hints of possible structural features, such as faint spiral arms or tidal tails, are present, but they are indistinct and may be artifacts of image resolution or processing. Overall, the galaxy seems to be a relatively smooth object with some indication of past or ongoing interactions. The light distribution suggests a mix of stellar populations, with older stars concentrated in the center and younger, bluer stars populating the outer regions.
