The galaxy presents as a centrally concentrated object with a moderate degree of morphological disturbance. Its overall color appears to be slightly blue-shifted, suggesting active star formation. The light profile is smooth with some features hinting to the presence of a spiral or disk component. There is evidence that this galaxy could be experiencing a minor disturbance, perhaps due to a past or ongoing interaction or accretion event. While the bulk of the galaxy appears relatively undisturbed, subtle asymmetries within the extended outer regions of the galaxy could indicate tidal interactions. The central bulge exhibits a diffuse morphology, not especially luminous, implying that any active galactic nucleus is likely low luminosity or obscured. Based on the color, luminosity, and features, it may be characterized as a moderately massive spiral galaxy with low-to-moderate star-forming activity.
