The galaxy appears as a centrally concentrated object with an overall elliptical morphology. There is a high degree of smoothness, with little evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits a yellowish-white color, suggesting an older stellar population. The shape is generally in between round and elongated, lacking a distinctly cigar-shaped appearance. There may be minor morphological disturbances, possibly indicative of past or ongoing interactions, however, a recent merger appears unlikely. The galaxy is moderately luminous. Star formation rates appear relatively low, in line with the galaxy's color and morphology.
