The galaxy appears to be a relatively compact object with a largely spheroidal morphology. It exhibits a smooth overall appearance with no obvious spiral arm structures or prominent dust lanes. Its color profile suggests a higher concentration of older stellar populations, emitting primarily in the redder wavelengths, although there is a bluer central region. The galaxy appears somewhat elongated, displaying a mild cigar shape. No evidence of significant tidal disturbances or ongoing major mergers is apparent. There is some indication of a minor asymmetry, potentially suggestive of a past or ongoing interaction, but this is not strongly pronounced. 
