The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is no apparent spiral arm structure or bar visible in this image. The light distribution suggests a nearly circular shape with a faint, extended halo. The color is slightly redder, indicating a population of older stars. There might be ongoing star formation, but it appears to be occurring at a relatively low rate. There is a suggestion of minor gravitational disturbance within the galaxy, but no strong evidence of a major merger event.
