The galaxy presents as a moderately luminous, disk-shaped structure, exhibiting an overall smooth appearance with some features. The central bulge is prominent and displays a concentrated yellowish hue, suggesting a population of older stars. The disk extending from the bulge shows a slightly bluer tint compared to the core, potentially indicative of ongoing star formation, albeit at a relatively low rate. The galaxy appears largely undisturbed, with only a subtle asymmetry possibly hinting at a minor interaction or disturbance. The round shape implies its more of a face-on galaxy, or possibly elliptical if there is no disk shape.
