The galaxy presents a largely smooth, elliptical morphology. It displays a centrally concentrated luminosity profile, indicating a significant bulge component. The color gradient suggests a population of older, redder stars dominating the central regions, while the outer regions may contain a mix of stellar populations. The galaxy shows little evidence of ongoing star formation based on its color and overall morphology. There are no apparent dust lanes or prominent spiral arms visible. The shape is generally round. No signs of recent major mergers or tidal disturbances are present.
