The object appears to be a galaxy, characterized by a centrally concentrated luminosity profile. The galaxy presents a generally smooth appearance, lacking prominent spiral arms or a well-defined disk structure. The light distribution exhibits a slight elongation, deviating from a perfectly circular morphology. The core region displays a yellowish hue, potentially indicating an older stellar population. Faint, diffuse extensions are observed surrounding the central region, though the low signal-to-noise makes detailed analysis challenging. There is no strong evidence of ongoing major merger activity or significant tidal disturbances. The morphology appears to be generally consistent with an elliptical galaxy or a lenticular galaxy viewed at a high inclination angle.
