The galaxy presents a generally smooth and elliptical morphology. Its light profile is centrally concentrated, with a bright core that gradually diffuses outwards. The object lacks any obvious spiral arm structures or distinct morphological features such as bars or rings. There is a slight elongation in its shape but it is generally roundish. The galaxy appears to be a relatively isolated system, lacking any strong visual evidence of ongoing major mergers or tidal disturbances. Its color indices suggest the presence of a fairly old stellar population.
