The galaxy presents as a moderately luminous, elongated structure with a smooth overall appearance. It appears elliptical in shape, with the major axis significantly longer than the minor axis. A central bulge is observed, exhibiting a yellowish hue suggestive of an older stellar population. The disk component displays a color gradient, appearing bluer towards the outer edges, potentially indicative of ongoing star formation. There is no obvious evidence of spiral arm structure or prominent dust lanes. The galaxy does not appear to be undergoing a major merger, although minor disturbances cannot be ruled out.
