The galaxy appears as a centrally concentrated, moderately luminous object with a smooth, somewhat elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars and a possible lack of significant ongoing star formation in the very central region. The outer regions of the galaxy display a gradual falloff in luminosity, transitioning to a fainter, more diffuse halo. There are hints of slight asymmetry, but no distinct spiral arms or strong tidal features are readily apparent in the image. The overall color profile suggests a mature stellar population throughout the galaxy, with little evidence of significant dust obscuration. The object appears to be relatively isolated, with no obvious signs of recent or ongoing interaction with other galaxies.
