The galaxy exhibits a relatively smooth morphology, with the majority of light concentrated in a central bulge. There's no prominent disk structure visible, but a very faint blueish object can be seen nearby, suggesting it may be a minor disturbance. The galaxy appears generally rounded in shape and the light is more yellow than blue. Based on the color index, this galaxy is likely composed of older stellar populations. There appears to be some evidence of recent or ongoing star formation, but it is likely to be relatively minor. The galaxy does not appear to be involved in any major mergers or significant tidal interactions based on its overall structure. It presents as a relatively isolated, evolved system.
