This galaxy presents a somewhat elliptical morphology, appearing mostly smooth in structure. The central region exhibits a concentrated luminosity with a yellowish hue, potentially indicative of an older stellar population. Moving outwards from the core, the color transitions to a bluer tone, suggesting the presence of a younger stellar population within the galaxy's outer regions. There is little evidence of spiral arms or significant dust lanes. Faint, slightly disturbed features are present in the outskirts. Based on its observed characteristics, this galaxy likely has a substantial stellar mass.
