The galaxy presents a predominantly smooth morphology with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Faint, diffuse features extend from the central region, indicating the presence of a disk or possibly tidal disturbances, although their structure is not clearly resolved. Some regions appear slightly bluer, implying ongoing star formation, but not at a high rate overall. There is some evidence of interaction or merging activity, shown by the slightly disturbed shape of the galaxy and the presence of minor asymmetric features. The roundness of the galaxy is not quite perfect and contains an in-between form. The galaxy appears to be undergoing some kind of disturbance.
