The galaxy presents a largely smooth, elliptical morphology. It exhibits a high degree of central concentration, appearing almost perfectly round with a slight elongation barely visible. There are no prominent spiral arms or bar structures detected. A faint, extended halo surrounds the central region, gradually fading into the background. The galaxy appears fairly homogenous in color, with a slight tendency towards redder hues, indicating an older stellar population with relatively low levels of ongoing star formation. No signs of significant tidal disturbances or interactions with neighboring galaxies are evident. The light profile appears consistent with an early-type galaxy, likely dominated by older stars.
