The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of roundness. A slight elongation is noted, but the overall shape approximates a spheroid. The light distribution appears fairly uniform across the galaxy's body, suggesting a lack of distinct spiral arms or other prominent structural features. Color indices indicate a population of older stars. Evidence for recent or ongoing star formation is subdued, with only subtle variations in color across the galactic disk. There are no apparent tidal tails or other signs of major recent merger events. However, there seems to be a slight visual disturbance present. Overall, the galaxy appears as a typical, evolved elliptical.
