The galaxy presents as a relatively small, elliptical-like structure. It exhibits a generally smooth morphology with a centrally concentrated luminosity profile. There is a slight elongation evident in the shape, suggesting it is not perfectly spherical and closer to a cigar shape. There is some evidence of bluer light within the galaxy, perhaps hinting at ongoing star formation. There is also a hint of some minor disturbance that may indicate past or current minor interaction with a smaller galaxy.
