The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge region, with a gradual decrease in surface brightness moving outwards. The color profile suggests a population of older stars, contributing to a slightly redder hue in the central regions, with perhaps some younger, bluer stars in the outer regions. There may be minor disturbances within the disk, but not any major indication of recent merger activity or strong tidal forces. The galaxy's overall morphology is neither perfectly round nor highly elongated, appearing somewhat in between.
