The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution exhibits a noticeable radial gradient, with the core appearing significantly brighter and more concentrated than the outer regions. There is little evidence of distinct spiral arms or prominent dust lanes. The overall color profile suggests an older stellar population, as indicated by the yellowish hue, but with a hint of bluer colors near the center, potentially indicating recent star formation. The shape is mostly round with a slightly elongated profile. There is no obvious signs of any major mergers or disturbances.
