This galaxy appears to be a relatively smooth, elliptical-type system, with little to no discernible spiral arm structure. The central bulge is quite prominent, exhibiting a high surface brightness and concentrated luminosity. The overall shape appears somewhat elongated but trending towards round, and it presents a generally even luminosity profile, indicative of an older stellar population and a possible lack of significant ongoing star formation. There might be signs of a minor gravitational interaction or disturbance exhibited as a very slight asymmetry in its form, however, further data is needed to establish certainty.
