The galaxy presents a moderately elliptical morphology. A smooth, centrally concentrated bulge dominates the overall light profile, surrounded by a more diffuse halo. The color gradient transitions from a slightly redder hue in the central regions to a bluer component in the outer parts of the disk. A subtle inclination is observed relative to our line of sight. There is no evidence of distinct spiral arm structure or significant dust lanes within the galaxy. Overall, the galaxy exhibits a relatively quiescent appearance, suggesting a lack of major recent merger activity.