The galaxy presents as a moderately inclined spiral or lenticular system, characterized by a central bulge that appears relatively smooth and luminous. The overall color gradient suggests a concentration of older stellar populations in the bulge, with a shift towards bluer hues in the surrounding disk. The disk component exhibits some structure, possibly indicative of spiral arms, although the image resolution limits a definitive assessment. The galaxy's shape is somewhat elongated and elliptical, rather than perfectly circular, with hints of minor disturbances in the disk. The overall light distribution is concentrated in the center, then tapers off into the edge of the galaxy. The galaxy does not appear to be undergoing any major merger activity, although there might be some minor interaction or disturbance influencing its morphology.
