The galaxy presents a smooth, elliptical morphology. Its light distribution is concentrated towards the center, appearing as a bright, yellowish core which gradually fades into a more diffuse outer region. The galaxy exhibits a somewhat elongated shape; possibly a cigar shape rather than perfectly spherical. There is no clear evidence of spiral arms or distinct features such as star clusters or dust lanes. The color profile suggests a relatively passive galaxy with a population of older stars, as indicated by the redder hues in the central region, although some bluer light is present in the outer parts. There appear to be no obvious signs of any major merging activity or significant disturbances. Any interaction appears to only be minor. The galaxy appears to be relatively isolated.
