The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated light distribution. It presents an elongated shape, with a cigar-like appearance. The galaxy's core exhibits the brightest luminosity, gradually fading outwards. There is no discernible spiral arm structure or obvious dust lanes, suggesting a lack of significant recent star formation. Based on the object's overall color, it seems dominated by an older stellar population. There is no clear evidence of a major ongoing merger event. Marginal disturbances or interactions may be present, but these do not severely disrupt the galaxy's primary morphology. Overall, the galaxy exhibits a relatively quiescent nature.
