The galaxy presents as a generally smooth object with a concentrated central region. The overall morphology appears elliptical, tending towards a round shape rather than a highly elongated form. The color profile suggests a relatively older stellar population, with a yellowish hue dominant in the core and extending outwards. There is minimal evidence of spiral arm structure or significant dust lanes. A faint, diffuse halo surrounds the brighter central region, gradually fading into the background. There are no obvious signs of tidal disturbances or major mergers; the galaxy seems relatively undisturbed. The absence of strong blue colors suggests a low rate of ongoing star formation.
