The galaxy presents a somewhat elliptical morphology with a smooth, featureless appearance. Its core region is characterized by a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Moving outward from the core, the luminosity gradually decreases, exhibiting a diffuse halo. The overall color profile leans towards the redder end of the spectrum, indicative of an older stellar population and potentially a reduced rate of star formation. There is no clear evidence of spiral arm structure, dust lanes, or significant tidal disturbances. The shape appears to be more in between round and cigar shaped than distinctly round. There may be a faint interaction with another galaxy but is difficult to tell based on the image. 
