This galaxy presents a moderately concentrated, elliptical morphology. The central bulge exhibits a yellowish hue, suggesting a population of older stars. There appears to be a faint, diffuse halo surrounding the galaxy. The color profile indicates a slightly bluer shift towards the outer edges, hinting at regions of ongoing star formation. There is evidence of minor disturbances or irregularities in the galaxy's structure, potentially indicating a recent or ongoing interaction with another galaxy. A subtle tidal feature might be present, although further data is needed to confirm this. Overall, the galaxy appears to be in a transitional phase, possibly evolving from a more disk-like structure towards a spheroid.
