The galaxy appears to be a relatively small, elliptical or lenticular galaxy with a smooth, diffuse structure. It exhibits a blue hue, possibly indicative of some ongoing, but relatively low, levels of star formation. The galaxy's morphology suggests it is mostly smooth, with no significant spiral arms or distinct features that would classify it as a spiral galaxy. The light distribution is concentrated towards the center, gradually fading towards the outer edges. There is some elongation in the galaxy's shape, tending toward a cigar-like appearance. There is an indication of some form of gravitational disturbance, with possibly a smaller object in the process of merging, or in close proximity, which is perhaps distorting the overall morphology of the galaxy. Overall, the galaxy gives the impression of a quiescent system, likely with an older stellar population.
