The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution suggests an absence of prominent spiral arms or a well-defined disk structure. The galaxy exhibits a relatively uniform color profile, with a slightly yellowish hue, which may indicate a population of older stars and a lower rate of ongoing star formation. The overall rounded shape suggests it is likely an elliptical galaxy viewed from a relatively face-on perspective. There is no visible evidence of any significant merging or tidal disturbances in its immediate vicinity.
