The galaxy presents an overall smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears approximately round. The color gradient transitions from a slightly redder hue in the core to a subtly bluer tint in the outer regions. There is no apparent evidence of spiral arm structure or significant dust lanes. The galaxy does not seem to be undergoing any major merging events or show signs of significant tidal disturbances in this image. The overall light distribution is relatively even and diffuse, without any prominent star forming knots or regions of intense blue light characteristic of young stellar populations. Its estimated size suggests that it is a medium sized galaxy.
