The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light distribution suggests a spheroidal component dominates the galaxy's structure, with little evidence of spiral arms or a distinct disk. Color gradients are present, with a yellowish-white core suggestive of an older stellar population, likely composed of Population II stars. Moving outwards from the center, a gradual transition to slightly bluer hues is visible, indicating the presence of some younger stars or regions of ongoing, albeit moderate, star formation.

There is no indication of strong tidal features, such as extended tails or bridges, that would be indicative of a recent major merger event. However, some subtle asymmetries in the outer regions might suggest minor gravitational interactions or past accretion events. The overall appearance aligns with that of an intermediate-mass galaxy with a relatively low star formation rate and a significant population of evolved stars.
