The galaxy presents a generally smooth morphology. It appears to be primarily elliptical or lenticular in nature, lacking the prominent spiral arms of a disk galaxy. The light distribution suggests a centrally concentrated bulge component. The galaxy has an intermediate ellipticity and does not look particularly round.

There is a slight asymmetry to the galaxy, suggesting a possible minor disturbance or interaction. This could be caused by a minor tidal effect from a past or ongoing interaction with a satellite galaxy, which is not clearly visible in the image. The color of the galaxy appears to be primarily red and green, indicating an older stellar population with relatively low recent star formation. It has an absolute magnitude comparable to that of other galaxies that would also fit this profile. 
