The galaxy presents as a single, relatively smooth object with a pronounced central bulge. The color profile suggests a population of older stars, likely with lower recent star formation. The overall shape is elongated, tending toward a cigar shape rather than a perfect sphere. There's no obvious spiral arm structure or significant dust lane obscuration visible, suggesting a possible classification as an elliptical galaxy. The relative smoothness of the galaxy supports this classification. There may be a minor interaction or tidal feature on the lower left, indicating past or ongoing gravitational interaction with a neighbor, but this could be the result of the poor image quality. The lack of strong blue colors, also suggests that there is no large amount of ionized Hydrogen gas in the galaxy. 
