The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests a relatively high degree of central concentration, with a gradual decrease in brightness moving outward from the core. The overall shape is generally rounded. There is little evidence of spiral arm structures or significant dust lanes. The color profile indicates a reddish-yellow hue overall, suggesting a stellar population dominated by older, redder stars and a low rate of ongoing star formation. The lack of significant blue regions indicates that the galaxy is not currently undergoing a major episode of star formation. There is no apparent sign of major mergers or tidal disturbances.
