This galaxy exhibits a generally smooth morphology, with a concentrated central bulge. There are limited discernible features such as spiral arms or a prominent disk structure. The galaxy appears somewhat elliptical, more so then spiral. Its color profile indicates a likely population of older stars, emitting primarily in the redder wavelengths of light. There is no clear sign of active star formation as denoted by the lack of intense blue color. No signs of ongoing or recent merger events are observed.
