This galaxy presents a predominantly smooth morphology. The overall shape appears to be somewhat elongated, presenting an intermediate shape between circular and a more cigar-like form. There is little evidence of significant spiral arm structure or prominent dust lanes. The central region exhibits a bright, concentrated core, suggesting a high density of stars or the potential presence of an active galactic nucleus, though this cannot be confirmed from this image alone. The outer regions show a gradual decrease in luminosity with indistinct edges. Faint reddish elements are loosely scattered throughout the galaxy, suggesting a potential population of older stars and some areas of current or past star formation. There does not appear to be any indication of an ongoing major merger event, but possible minor disturbances or tidal features cannot be entirely ruled out based solely on this image. The galaxy appears to be a relatively isolated system in this field.
