The galaxy presents as a relatively smooth, elliptical-like structure. Its morphology leans toward a rounded shape, with the isophotes exhibiting only a slight deviation from circularity. The color profile indicates a population of older stars, with a redder hue dominating the central regions and a very slight hint of blue in the outer regions. There is no apparent spiral arm structure or prominent dust lanes. No significant tidal features or signs of major mergers are immediately obvious, though a minor disturbance cannot be ruled out due to the slight irregularity in the overall shape. The galaxy appears fairly compact, indicating a high concentration of stellar mass within a small radius.
