This galaxy presents as a slightly elongated, lenticular-like structure. It has a relatively smooth and diffuse appearance, with a brighter central region that gradually fades towards its periphery. The galaxy appears to be moderately blue-shifted, suggestive of younger stellar populations. There is a distinct lack of well-defined spiral arms or prominent dust lanes, indicating a system with potentially limited ongoing star formation, though the blue color could indicate some presence of star formation activity. The overall shape is somewhat cigar-shaped, with a smooth transition in brightness across its extent. There are no obvious signs of a major merger event, though some minor disturbances may be present based on the slight irregularities in its overall form. The galaxy’s light is consistent with that of a medium-mass galaxy.
