The galaxy presents an elliptical morphology, elongated along its major axis, suggesting an E4-E6 classification on the Hubble sequence. The central bulge appears prominent and exhibits a smooth, concentrated brightness profile, indicative of an older stellar population. The surrounding disk or halo is less defined, displaying a fainter, more diffuse glow. There are no readily apparent spiral arm structures or significant dust lanes. The overall color profile suggests a redder hue, consistent with a population of older stars and a relatively low rate of ongoing star formation. The galaxy appears relatively undisturbed, showing no obvious signs of recent merger activity.
