The galaxy appears as a single, relatively smooth structure, with little to no visible spiral arm detail or distinct morphological features, such as bars or rings. The overall shape is close to circular, exhibiting only a slight ellipticity. The light distribution is centrally concentrated, with a bright core that gradually fades into the surrounding halo. The color gradient suggests a population of older stars. The color composite of the galaxy reveals a generally yellow hue, with hints of redder tones towards the outer regions. This color suggests that the galaxy is composed of a significant population of older stars and a relatively low amount of ongoing star formation. There is no evidence of any major disturbances or ongoing mergers. The light is quite diffuse.