The galaxy presents a generally smooth and concentrated morphology. The central region is a bright, yellowish-white core that diminishes in intensity towards the outer regions. There's a slight elongation suggesting a departure from perfect circularity, although it doesn't appear strongly barred or elliptical. Some faint, diffuse extensions surround the central body, but no distinct spiral arm structures or prominent features like dust lanes are discernible. There might be minor disturbances in the outer halo, but no signs of any major mergers or collisions. The galaxy's overall color profile suggests a population of older stars and a relatively low rate of on-going star formation.
