The galaxy presents an overall smooth morphology, with a dominant spheroidal component. The central region appears more concentrated and exhibits a reddish hue, possibly indicating an older stellar population. The isophotes appear elliptical rather than perfectly circular. Fainter, bluish light extends outwards from the core, suggesting the presence of a younger stellar population compared to the nucleus. Possible minor disturbances are visible in the extended outer regions. There may be an indication of a disk structure.
