The galaxy presents a relatively smooth morphology, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. The surrounding disk appears somewhat diffuse and less structured, fading into the background. Hints of bluer star formation regions are subtly present within the outer regions of the galaxy, though not prominently defined. The overall shape is moderately elliptical, with a slight elongation along its major axis. There is no obvious evidence of strong tidal interactions or ongoing merger activity. 
