The galaxy presents as an elliptical morphology, with a high degree of central concentration. The light profile appears smooth, with no visible spiral arm structure or prominent dust lanes. The galaxy exhibits a moderate degree of ellipticity, appearing more oval than perfectly spherical, tending toward a cigar shape. There's a distinct color gradient, with the central region appearing more yellowish, possibly indicative of an older stellar population and lower levels of ongoing star formation. The outer regions exhibit a bluer hue, suggesting the presence of some younger stars, though at a lower overall rate. There is no evidence of any major merging events or significant tidal disturbances in the immediate vicinity of the galaxy. The overall structure indicates a gravitationally relaxed system, likely a mature galaxy.
