The galaxy presents as a relatively smooth, elongated structure. There's a noticeable central bulge, appearing more concentrated in light intensity than the outer regions. This suggests a higher density of older stars within the galactic nucleus. Fainter, diffuse extensions are observed extending from the central bulge. These extensions show a hint of bluer light, possibly indicating regions of more recent, though still relatively subdued, star formation. The overall morphology leans towards a classification between elliptical and lenticular, showing characteristics of both in terms of smoothness and disc-like structure. There are no clear signs of major recent merger activity, though subtle disturbances or tidal features cannot be ruled out entirely given the limited image resolution. The galaxy's moderate redshift indicates that it is not a nearby galaxy. It is not highly luminous, and may be a dwarf galaxy.
