The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, with an approximate Petrosian half-light radius of 9 kpc. The galaxy exhibits a yellowish hue, suggesting an older stellar population and a relative lack of ongoing star formation activity. There is no evident spiral structure or prominent dust lanes. The overall color profile indicates a dominant population of evolved stars, with a low specific star formation rate. It seems undisturbed, without any obvious signs of ongoing or recent merger events. The galaxy is approximately round in shape, and does not seem to be part of any larger group or cluster based on its immediate surroundings.
