The galaxy presents as a primarily smooth object, exhibiting a concentrated central bulge that graduates outwards into a less defined disc. The colour profile suggests an older stellar population, with a yellowish hue dominating the central regions. There is a possible slight reddish trend towards the outer edges, perhaps indicative of dust.

The galaxy appears to be relatively isolated, showing no immediately apparent signs of interaction with other galaxies or tidal disturbances, maintaining a largely undisturbed morphology. The galaxy appears neither particularly disc-like, nor especially spheroidal, suggesting that it may fall between elliptical and spiral classifications.
