This galaxy exhibits a relatively smooth morphology, appearing elliptical or lenticular in shape. A dominant, bright central bulge is visible. There are no prominent spiral arms or significant dust lanes observed in this image. The overall color profile suggests a population of older stars, with a slightly redder hue in comparison to galaxies with ongoing star formation. There are no apparent signs of recent or major merger activity. The galaxy appears to be well-defined, with a smooth transition from the central bulge to the outer regions. The color gradient suggests a relatively even distribution of stellar populations. The galaxy exhibits an overall round shape, with a slight deviation towards a more elongated form. There is a minimal amount of disturbance observed.