The galaxy presents as a lenticular or cigar-shaped object. It exhibits a smooth, somewhat diffuse morphology, suggesting a lack of prominent spiral arms or significant irregular features. The light distribution is concentrated centrally, diminishing outwards.

The color appears to be primarily a yellowish hue, potentially indicative of an older stellar population. There is no strong indication of blue light which would otherwise suggest intense, recent star formation. It is possible that the galaxy is undergoing relatively low levels of star formation. There is no obvious presence of any major ongoing merger activity or interaction with other galaxies, although there are subtle disturbances.
