The galaxy presents as a largely elliptical morphology, with a high degree of central concentration. The light distribution appears smooth with no prominent spiral arms or distinct features, suggesting an older stellar population. The galaxy's color is primarily yellow-orange in the central region, possibly indicating a bulge dominated by evolved stars, with subtle reddish hues that could indicate dust extinction or regions of ongoing star formation. The outer regions of the galaxy appear fainter, and are a mottled greenish blue, consistent with a degree of star formation. The isophotes are generally round to slightly elliptical, but there is no obvious evidence of a major ongoing merger or significant tidal disturbance, though a very slight asymmetry in the outer region is suggestive of past gravitational interaction.
