This galaxy presents as a concentrated central bulge exhibiting a strong yellow-orange hue, indicative of an older stellar population. The galaxy lacks well-defined spiral arm structures. A faint and diffuse disk surrounds the central bulge, with a subtle color gradient suggesting it is bluer than the bulge, which may indicate pockets of more recent star formation. The overall morphology suggests a possible elliptical or lenticular galaxy type, exhibiting a smooth light profile. There is no apparent strong tidal interaction or major merger activity occurring, with only a slight asymmetry in the outer disk suggesting a potential minor disturbance. The galaxy appears to be relatively isolated in its environment. 
