The galaxy presents a predominantly smooth morphology, with a concentrated central bulge that appears yellow-orange in color. The light distribution from the core diffuses outwards, decreasing in intensity with radial distance. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes, indicative of a relatively uniform stellar population. The overall shape is neither perfectly spherical nor highly elongated, suggesting an intermediate ellipticity. Faint, diffuse light extends beyond the central region, creating a halo-like effect. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances.
