The galaxy appears as a slightly elongated, disk-shaped structure with a smooth, diffuse light distribution. There is a bright, concentrated core region that appears nearly spherical. The isophotes appear elliptical, with a tilt towards the upper left of the image, suggesting a possible inclination relative to our line of sight. The overall color is consistent with a relatively older stellar population, with a somewhat bluer core. No distinct spiral arm structures or prominent dust lanes are discernible at this resolution. The galaxy seems to be relatively isolated, with no obvious signs of ongoing major mergers or strong tidal interactions with other galaxies. However, some minor disturbances are possible.
