The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution with a central bulge dominating the visual appearance. The galaxy is elongated in shape, showing a cigar-like form with a high degree of central concentration. There is no evident spiral structure or distinct disk component visible at this resolution. The color profile suggests a population of older stars, with a reddish hue prevailing across the galaxy's extent. There is no evidence of ongoing major merger activity or significant tidal disturbances, although a very slight asymmetry might indicate a minor interaction in the past. Star formation rates are likely low.
