The galaxy presents as a concentrated, elliptical morphology, with a high degree of central light concentration, suggestive of an older stellar population. The color profile is generally consistent, with a slight reddening towards the central regions, possibly indicating a lack of recent star formation there. The disk is subtly visible, but it is not a distinct feature of the galaxy. Any spiral arms cannot be distinguished.

Based on the galaxy's color and morphology, this appears to be a fairly massive and evolved galaxy. There is no significant evidence of tidal disturbances or major mergers in the immediate vicinity.
