The galaxy presents as a somewhat amorphous, slightly elongated structure, exhibiting a smooth light distribution. It appears to be relatively compact. A central, brighter region suggests a concentration of stellar density, possibly a galactic bulge or active galactic nucleus. Faint, diffuse extensions are observed around the central region, hinting at a more extended halo or envelope. The overall color is a yellowish-white, indicating a mix of stellar populations with perhaps a predominance of older stars, given the redder hue. Subtle color variations within the galaxy suggest possible differences in stellar populations or dust content across the galaxy's body. There is little evidence of spiral arms or distinct morphological features, suggesting a later-type galaxy.
