The galaxy appears as a centrally concentrated object with a generally smooth morphology. Its shape is predominantly round with some features in the disk. There is evidence of some disturbances within the galaxy, but they are not classified as major mergers or significant tidal interactions. The galaxy's central region exhibits a reddish hue, transitioning to bluer tones in the outer regions. The light distribution appears consistent, suggesting a relatively evolved stellar population with an older population dominating. There is little to no indication of active star formation within this galaxy.
