The galaxy presents as a moderately luminous, elongated structure. Its overall form leans towards spheroidal but exhibits a subtle disk-like component. The central region displays a concentrated, bright core, suggesting a relatively high stellar density. The galaxy's color profile is primarily a pale yellow-white, indicative of an older stellar population with a lower rate of current star formation. Some faint blue tinges are noticeable, potentially indicating regions of younger stars, although these are minimal. There is little to no evidence of strong spiral arm structures or significant dust lanes within the galaxy. There appears to be some minor distortion in the overall shape, indicating possible interaction.
