The galaxy appears as a smooth, elongated structure, with a cigar-like shape. The light is concentrated towards the center, suggesting a high central density. There is a color gradient visible, with the central region appearing more yellow, likely due to an older stellar population. The outer regions exhibit a reddish hue, which could indicate dust or the presence of cooler, older stars. There is no obvious evidence of spiral arms or a well-defined disk structure within the resolution limits. The galaxy does not appear to be undergoing a major merging event, although there is a minor asymmetry which could indicate a minor interaction. Overall, the galaxy presents characteristics consistent with an elliptical galaxy.
