The galaxy presents as a centrally concentrated, relatively smooth object. The core exhibits a bright, diffuse glow, transitioning outwards to a fainter, more extended halo. The galaxy appears roughly elliptical, though not perfectly circular. There is a slight elongation. Based on the color profile, the galaxy's stellar population consists of a mix of younger, bluer stars in the core region, and older, redder stars concentrated in the outer regions. There is no apparent spiral structure or strong dust lane obscuration visible. The lack of significant morphological disturbances suggests the galaxy has not undergone a recent major merger. Minor irregularities and deviations from perfect symmetry within the fainter outer halo are present, perhaps indicating a history of minor accretion events or some form of tidal interaction. Overall, the galaxy's morphology is suggestive of an early-type galaxy, possibly an elliptical or lenticular.
