This galaxy appears as a relatively compact, somewhat smooth object. A concentrated central bulge is observed, exhibiting a bright, predominantly blue-white coloration. This coloration suggests the presence of a significant population of young, hot stars within the core. There is some indication of asymmetry in the outer regions, potentially hinting at a minor gravitational interaction or disturbance. A faint, diffuse halo surrounds the central structure, with some subtle irregularities detectable at the periphery. The overall morphology leans towards a more elliptical shape, though a definitive classification is challenging due to the limited resolution and potential disturbances.
