The galaxy appears as a moderately luminous, elongated structure. A dominant central bulge is observed, exhibiting a smooth, concentrated brightness profile, suggestive of an older stellar population. Extending outwards from the bulge, a faint and diffuse disk is visible. The disk appears to be inclined relative to our line of sight, contributing to the galaxy's elliptical shape. There are no prominent spiral arm structures discernible. Subtle color gradients are observed, with the central bulge displaying a more yellowish hue, potentially indicative of older stars and lower levels of ongoing star formation compared to the bluer colors in the disk. There is no evidence of any major merger events or significant tidal disturbances. The overall morphology appears relatively undisturbed.