The galaxy presents as a roughly elliptical, though somewhat irregular, structure. The central region exhibits a concentrated, bright luminosity, appearing yellowish-orange. This suggests a high density of older stellar populations and potentially a significant presence of dust. Fainter, bluer hues are observed towards the outer edges, possibly indicative of more recent star formation in those regions, although this activity appears subdued. The overall morphology suggests an intermediate stage between a pure elliptical and a spiral galaxy, perhaps a lenticular (S0) type or a spiral undergoing transformation into an elliptical. There is a slight asymmetry in the distribution of light, suggesting a possible interaction or past merger event. There's no clear evidence of strong tidal features or a prominent disk structure, which further supports its classification closer to the elliptical end of the galaxy morphological spectrum.
