The galaxy presents a largely smooth and rounded morphology, appearing elliptical in form. There is a concentrated central bulge exhibiting a bright, yellowish-white hue, indicative of an older stellar population. Fainter, diffuse light extends outwards from the core, with a slight elongation perceptible along one axis. There appears to be little to no discernible spiral structure. Any faint, slightly bluish light surrounding the core of the galaxy might indicate regions of recent star formation. There is no obvious evidence of significant tidal disturbances, major mergers, or other features that might suggest strong gravitational interactions. Based on visual assessment of the data, the galaxy is likely a quiescent elliptical galaxy with a relatively low star formation rate.
