The galaxy presents a relatively smooth and concentrated morphology. The light distribution suggests an elliptical or lenticular classification, potentially leaning towards the latter given the slightly elongated shape. There is a bright, concentrated core with a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy exhibit a bluer tint, suggesting the presence of some younger stars and/or ongoing star formation, although this activity appears to be subdued. The galaxy's overall structure appears undisturbed, with no obvious signs of recent major merger events. Faint, extended halos or tidal features are not readily apparent, suggesting a relatively isolated evolutionary path. The axial ratio implies a significant inclination with respect to our line of sight, though not edge-on.
