The galaxy presents a moderately elongated morphology, appearing more cigar-shaped than circular. The light distribution suggests a relatively smooth structure with a central concentration. There is a subtle color gradient observed, with a yellowish core potentially indicating a population of older stars, while the outer regions exhibit a bluer tint, possibly indicative of ongoing or recent star formation activity. No distinct spiral arms or prominent dust lanes are discernible. The overall appearance is suggestive of a galaxy undergoing moderate levels of star formation within a somewhat evolved stellar population, without evidence of major mergers or significant tidal disturbances.
