The galaxy appears as a lenticular or possibly an elliptical galaxy, exhibiting a smooth, centrally concentrated luminosity profile. It presents an elongated morphology, appearing cigar-shaped, with an ellipticity that indicates it is viewed at an angle. The central region is brighter and yellower, indicative of an older stellar population, possibly dominated by evolved red giant stars and a lack of significant recent star formation. The galaxy shows no obvious spiral arm structure or prominent dust lanes. Faint blue tinges are present in the galaxy outskirts, possibly indicating a small population of younger, hotter stars, but are not pronounced. There is no clear evidence of a major ongoing merger event or significant tidal disturbance. The overall color suggests a relatively passive galaxy, consistent with a low specific star formation rate.
