The galaxy presents a largely smooth morphology, with a centrally concentrated, bright core. There is little evidence of spiral arms or other distinct features. The galaxy appears elliptical or lenticular in shape, exhibiting a high degree of central symmetry. The color profile suggests a primarily older stellar population, with a yellowish hue dominating the core and inner regions. The outer regions show a slightly bluer tint, possibly indicating a small amount of ongoing star formation, although the overall star formation rate appears to be relatively low. There are no obvious signs of a major merger event or significant tidal disturbances. The galaxy displays an intermediate axis ratio, appearing slightly elongated, but not highly flattened.
