The galaxy presents as a concentrated, elliptical form, exhibiting a generally smooth morphology. The core displays a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards, the color profile shifts towards a redder tone at the edges of the galaxy, possibly indicating a lower rate of star formation compared to the core, and a higher percentage of older stars.

There is no obvious spiral arm structure, but some subtle asymmetry is present in the outer regions, potentially indicative of a minor interaction or past merger event. No significant dust lanes are visible. The galaxy's concentrated morphology and color profile support its classification as a galaxy with a smooth appearance. The redder outer regions further suggests an older stellar population.
