The galaxy presents a generally smooth morphology. The central region exhibits a high degree of concentration, appearing as a bright, slightly oblong spheroid. The galaxy's color profile trends towards the redder end of the spectrum, suggesting a population dominated by older stars and a relatively low rate of current star formation. There is little evidence of prominent spiral arm structures or significant dust lanes. A subtle asymmetry is observed in the outer regions, possibly indicative of a minor interaction or past merger event. Overall, the galaxy appears to be a relatively massive, quiescent system.
