The galaxy presents a generally smooth, elliptical morphology with a noticeable lack of distinct spiral arm structures. Its overall shape is elongated, approximating a cigar-like form. The core exhibits a high degree of central concentration, appearing as a bright, relatively uniform region. There is a gradual decrease in luminosity moving outwards from the core, transitioning into a faint, diffuse halo. The color profile suggests a population of older stars, with a general lack of intense blue hues indicative of ongoing, significant star formation. There may be some subtle signs of minor tidal disturbances or interactions, indicated by slight asymmetries in the outer halo. These potential disturbances do not appear to be indicative of a major ongoing merger. The galaxy presents a moderately low specific star formation rate, suggesting the galaxy's stellar mass is not undergoing rapid growth from star formation. 
