The galaxy presents as a smooth, elongated structure, consistent with an elliptical morphology. The central region exhibits a higher surface brightness, appearing more concentrated. The galaxy's color profile indicates a population of older stars, contributing to its overall redder hue. There is no apparent spiral structure or active star formation visible. The galaxy is relatively isolated, showing no obvious signs of interaction or tidal disturbances with neighboring galaxies. The overall smooth texture suggests a lack of significant dust lanes or prominent features associated with younger stellar populations. The major axis is clearly defined, with a gradually decreasing surface brightness towards the outer edges of the galaxy. The overall structure suggests a relatively evolved system, possibly residing in a region of lower galaxy density.
