The galaxy presents an elliptical morphology, appearing largely smooth and devoid of prominent spiral arm structures. The central region exhibits a concentrated luminosity, indicating a significant stellar density. This core gradually diminishes in brightness towards the outer edges, suggesting a radial decline in stellar population density. The galaxy’s color profile leans towards redder hues, indicative of an older stellar population dominated by red giant stars, with a correspondingly low rate of ongoing star formation. There is no clear indication of significant tidal disturbances or recent major merger events in the immediate vicinity, as the galaxy appears relatively undisturbed. The overall structure is fairly uniform, lacking distinct features such as dust lanes or prominent star-forming regions. The axial ratio suggests the galaxy is more elongated than perfectly circular.