The galaxy appears as a centrally concentrated object with an overall elliptical morphology. The light distribution is relatively smooth. The color suggests an older stellar population, with a dominant yellow hue. There is some evidence of an adjacent object potentially interacting with the primary galaxy, exhibiting a bluer color, which may indicate ongoing star formation. There is no strong dust lane structure or prominent spiral arm features visible. Given the smooth appearance and redder colors, the galaxy is likely an early-type galaxy with a quiescent star formation rate. There seems to be an indication of some disturbed morphology, possibly due to gravitational interaction or a minor merger event.
