The galaxy presents as a relatively smooth, elliptical form with a concentrated central bulge. The overall color profile suggests a population dominated by older stars, trending toward the redder end of the spectrum. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears to be in a state of merger, likely having interacted with another galaxy in the past. The lack of defined structures might reflect a recent coalescence. There appears to be some tidal disruption, but it may be difficult to verify visually due to the viewing angle and distance. The galaxy exhibits an apparent spheroid shape.