The galaxy presents an overall elliptical morphology, although some irregularities are apparent. A centrally concentrated bulge region dominates the light profile, appearing smooth and yellowish, suggesting an older stellar population. Fainter, more diffuse emission extends outward from the bulge along the major axis, potentially indicating a flattened disk structure. Some subtle features, such as faint wisps or arms, are possibly present within the disk. The galaxy's color suggests a relatively low rate of star formation and a stellar population dominated by older, redder stars. No obvious signs of a major merger are readily apparent, although minor tidal disturbances cannot be ruled out. The galaxy exhibits a moderately inclined orientation with respect to our line of sight. Overall the galaxy appears to be a relatively massive system.