The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology with no obvious spiral arm structure. The light distribution suggests an elliptical or lenticular galaxy classification. There is a slight elongation evident, deviating from a perfectly circular profile. 

There appears to be a very minor disruption, possibly a small tidal feature or asymmetry suggesting a past or ongoing minor interaction or accretion event. The galaxy displays a relatively homogenous color profile across its body. There is no distinct bright galactic nucleus.
