The galaxy presents a roughly elliptical morphology, displaying a moderate degree of flattening. The central region exhibits a concentrated luminosity profile, appearing as a bright, yellowish core. Moving outwards from the core, the light becomes more diffuse, showing a subtle transition into a less structured disc or halo. Evidence of spiral arms is not readily apparent. The overall color profile suggests a population dominated by older stars, with lower rates of active star formation. There are indications of some disturbances within the disc, such as minor asymmetries or faint tidal features, that imply recent or ongoing interactions. These disturbances are not severe enough to classify it as a major merger event. The galaxy is neither perfectly circular nor elongated but falls somewhere in between.