The galaxy presents an elliptical morphology, exhibiting a centrally concentrated luminosity profile. A bulge is clearly visible, characterized by a smooth, diffuse glow that dominates the inner region. The galaxy appears generally featureless, lacking prominent spiral arms or distinct dust lanes in this image. There is a slight elongation of the galaxy along a major axis oriented approximately east-west. The color gradient suggests a population of older stars, with the core appearing more yellowish-red than the outer regions. The relatively smooth appearance indicates a high likelihood of being an early-type galaxy, specifically an elliptical, in a relatively relaxed state, possibly nearing a cessation of star formation. There is no obvious evidence of recent or ongoing merger activity.
