The galaxy presents an elliptical morphology, appearing elongated in shape with a high degree of smoothness. The central bulge exhibits a bright, concentrated luminosity, suggesting a dense stellar population. Moving outward from the bulge, the luminosity gradually decreases. The color profile indicates a relatively redder hue overall, implying an older stellar population and a possible dearth of ongoing star formation within the galaxy. Faint hints of a disk structure may be present, but any spiral arm features are either absent or not clearly discernible at this resolution. There is no evident indication of any major merging activity or significant tidal disturbances, but there could be signs of minor disturbances.
