The galaxy presents as a largely featureless, elliptical morphology. It exhibits a high degree of central concentration, with the light intensity gradually decreasing from the core outwards. The galaxy appears to be dominated by an older stellar population, suggested by its yellowish hue, indicating a lower rate of recent star formation. There is no clear evidence of spiral arms, a prominent disk, or ongoing major merger activity. Subtle disturbances could be present, but are not readily apparent from this image. The overall impression is that of a mature, relatively quiescent galaxy.
