The galaxy presents a generally smooth morphology, appearing elliptical in shape. The light distribution is concentrated towards the center, exhibiting a bright, relatively symmetric core. A subtle color gradient suggests a possible aging stellar population with a dominant yellowish hue. While a faint, extended halo may be present, there is little evidence of distinct spiral arms or significant star formation regions visible in this image. Subtle disturbances may be present, possibly indicating a minor interaction or past merger event. The galaxy appears to be largely quiescent in terms of star formation activity.